Priorities are defined for the TSO WG:
1: Critical — will produce unusable results for TSOs.
2: High — will produce sub-optimal results for TSOs.
3: Low — will produce slightly offset results for TSOS.
|Proposed enhancement||Brief description||TODOs||Relevant jira ticket (s)||Meeting links where this was discussed||Status||Priority||Update date|
|TSO3 Outlier Detection|
Currently, the JWST pipeline does not properly use TSO information to reject outliers (e.g., jump step or current tso3 outlier rejection — see Jira tickets). Proposed to implement HST/STIS algorithm developed by Nikolay Nikolov on JWST TSO pipeline.
Problems with current TSO3 step:
|CalWebb WG: 2021-05-04 Meeting Notes; 2021-01-05 Meeting Notes.|
TSO WG: 2021-02-24 TSO WG Meeting notes.
|3||December 2, 2021|
|Jump detection using TSO information|
Similar to the above, but do it at the group-level; detect jumps using TSO information. This is an idea proposed by Michael Regan. Pros: you don't rely on the reference files.
|Correct jitter spectral movement prior to photom step||If jitter is an issue during JWST observations, then the photom step will incorrectly apply photometric flux standarization to the wrong wavelengths, introducing time-dependant systematics. TSO WG reps think turning off the photom step would be ideal, but not generic solution. Correcting those jitters prior to the photom step would be a solution.|
CalWebb WG: 2021-06-01 Meeting Notes.
TSO WG: 2021-06-02 TSO WG Meeting notes.
|Spectral tracing||Pipeline needs to perform spectral tracing of TSOs in order to (a) record trace movements (useful as external parameters to decorrelate lightcurves) and (b) extract the same portion of the spectrum at each time.|
|2||December 15, 2021|
|Photometric Centroiding||Same as spectral tracing, but for photometry.||2|
|Pre-amp reset correction ("reference pixels for subarrays without reference pixels")|
|1||January 3, 2022|
|2||January 3, 2022|
|2||January 3, 2022|
Discussion on this:
|1||December 15, 2021|
|Integration-level aperture positions|